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HAT-P-28
Star in the constellation Andromeda From Wikipedia, the free encyclopedia
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HAT-P-28 is the primary of a binary star system about 1320 light-years away. It is a G-type main-sequence star. The star's age is older than the Sun's at 6.1+2.6
−1.9 billion years.[3] HAT-P-28 is slightly enriched in heavy elements, having a 130% concentration of iron compared to the Sun. Evolutionary modelling shows it to be right at the end of its main sequence life.[2] The binary star system is suspected to be surrounded by a debris disk with a 6.1″(2500 AU) radius.[7]
The red dwarf stellar companion was detected in 2015 at a projected separation of 0.972″[8] and confirmed in 2016 to be either bound or co-moving.[5]
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Planetary system
In 2011 a transiting hot Jupiter planet b was detected on a nearly circular orbit. The planetary equilibrium temperature is 1,384±52 K.[3] No orbital decay was detected as in 2018, despite the close proximity of the planet to the host star.[6]
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References
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